Trough in the daytime F layer: A macroscopic effect of ionospheric-magnetospheric convection
The daytime F layer trough is a major result of ionospheric-magnetospheric convection, appearing in the winter high latitude ionosphere as a continuous band thousands of kilometers in extent in which the daytime F layer electron density is depleted, often by an order of magnitude. As observed by a global array of ionospheric sounders during solar maximum, the trough occurs in regions of sunward convection, in the morning corresponding to the dawn cell and in the afternoon corresponding to the dusk cell. The formation of the trough is consistent with the transport of low density nighttime plasma into the day sector where it displaces high density daytime plasma, although other mechanisms such as ion chemical effects may also play a role.
- Research Organization:
- Air Force Geophysics Lab., Hanscom AFB, MA (United States)
- OSTI ID:
- 6193479
- Report Number(s):
- AD-P-006270/3/XAB
- Resource Relation:
- Other Information: This article is from 'The Effect of the Ionosphere on Radiowave Signals and Systems Performance Based on Ionospheric Effects Symposium Held on 1-3 May 1990', AD-A233 797, p60-68
- Country of Publication:
- United States
- Language:
- English
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Daytime F-layer trough
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Related Subjects
GENERAL PHYSICS
F REGION
ELECTRON DENSITY
AURORAL OVAL
CONVECTION
DAILY VARIATIONS
DISTURBANCES
EARTH MAGNETOSPHERE
INTERACTIONS
IONOSPHERE
LATITUDE EFFECT
PLASMA DENSITY
PLASMA DRIFT
EARTH ATMOSPHERE
ENERGY TRANSFER
GEOGRAPHICAL VARIATIONS
HEAT TRANSFER
MASS TRANSFER
PLANETARY IONOSPHERES
VARIATIONS
661320* - Auroral
Ionospheric
& Magnetospheric Phenomena- (1992-)